English

Dark matter searches with a 13 meV threshold superconducting sensor array

High Energy Physics - Experiment 2026-07-21 v1 Instrumentation and Methods for Astrophysics Quantum Physics

Abstract

Many well-motivated dark matter models predict meV-scale energy deposits in interactions with terrestrial experiments, but this regime is challenging to probe due to a lack of mature single-quantum detectors. Here we report results from QUALIPHIDE (QUAntum LImited PHotons In the Dark Experiment), a cryogenic dark matter search using a 4141-pixel array of energy-resolving microwave kinetic inductance detectors with a 1313 meV threshold, simultaneously used to look for both conversion photons from THz wavelength hidden photon dark matter and phonons from particle-like light dark matter interactions. The experimental design, with on- and off-focus pixels for the hidden photon search, allows for a data-driven background model, giving the experiment discovery potential. A blind analysis of 2222 hours of data shows no significant excess, setting the strongest constraints on the hidden photon kinetic mixing parameter χ\chi over the mass range of 1313-9090 meV/c2c^2, reaching 1.5×10121.5\times10^{-12} at 5050 meV/c2c^2. These data also yield among the first terrestrial limits on dark matter scattering off nuclei and electrons, down to 55 MeV/c2c^2 and 2020 keV/c2c^2, respectively. The low threshold also enables future study of the low-energy excess limiting cryogenic detectors and, as we project, will allow for a terahertz-scale QCD axion search with a magnetic field.

Cite

@article{arxiv.2607.19319,
  title  = {Dark matter searches with a 13 meV threshold superconducting sensor array},
  author = {Christopher Albert and Lanqing Yuan and Jacob Harris and Ritoban Basu Thakur and Andrew Bear and Karl K. Berggren and Christopher Cappiello and Christopher Curwen and Peter Day and Byeong H. Eom and Arjun Ghosh and William Ho and Nikita Klimovich and Henry G. LeDuc and Karthik Ramanathan and Alejandro Simon},
  journal= {arXiv preprint arXiv:2607.19319},
  year   = {2026}
}
R2 v1 2026-07-22T20:51:00.770Z